干旱区梨园不同覆盖条件下土壤环境因子综合性评价研究

在干旱沿黄灌区开展不同覆盖材料配合滴灌的灌溉保墒方式下,进一步研究了不同覆盖方式对梨园全生育期的土壤理化性状和养分含量变化影响,分析了土壤温度、水分、pH等和矿质营养元素间的相互关系,对覆盖后的土壤质量进行了综合性评价。试验处理分为无覆盖对照（T1）、园艺地布覆盖（T2）、玉米秸秆覆盖（T3）和黑地膜覆盖（T4）4个处理;试验设计为随机区组设计,每个处理小区均为167株梨树（约占地667 m²）,重复3次;各小区土样分0~20 cm、20~40 cm、40~60 cm土层取样。结果表明：（1） 园艺地布和黑地膜覆盖处理有一定的增温效应,而玉米秸秆覆盖有较好的降温和稳温效应,且增墒效应明显,土壤含水率比其他3种处理显著提高了1.0%~2.7%。（2） 相较无覆盖处理,黑地膜覆盖可提升表层土壤pH,并加速表层土壤有机质的分解,有机质含量较无覆盖处理下降33.1%;玉米秸秆覆盖可显著降低各土层的土壤pH,降低范围为1.8%~4.6%,并促进0~20 cm土层有机质的提升,土壤有机质含量增加12.2%;园艺地布覆盖下0~40 cm土层内土壤有机质含量和全盐量均有降低。（3） 黑地膜覆盖下0~20 cm和20~40 cm土层的碱解氮含量分别为73.00 mg·g^-1和64.53 mg·g^-1,均显著地高于无覆盖处理,无覆盖条件下土壤碱解氮在深层（40~60 cm土层）积累较多,显著地高于玉米秸秆和黑地膜覆盖;各处理0~20 cm和20~40 cm土层速效磷含量差异显著,大小顺序均为T4>T3>T2>T1,玉米秸秆覆盖可提升土壤速效钾和速效铁的含量。（4） 进行主成分分析表明不同覆盖方式对梨园浅层土壤环境因子的影响要明显大于深层土壤,在0~40 cm土层内各覆盖处理效果均好于无覆盖处理,其中玉米秸秆覆盖在0~20 cm和20~40 cm土层综合得分分别为1.189和0.326,覆盖效果最佳。     

GPS/BDS组合系统伪距单点定位模型精度分析

合理确定观测值权阵对于应用GPS/BDS组合系统提高单点定位的精度和稳定性十分重要.文章对GPS/BDS常用的几种定权模型等权模型、高度角随机模型、基于Helmert验后方差估计模型、顾及PDOP值的定权模型等进行了实验与分析.结果表明:基于Helmert的定权方法精度最高,进一步对其观测值的分类根据高度角进行改进并利用PDOP值的选星思想后,模型精度再次提高.研究结果可以为提高GPS/BDS组合系统伪距单点定位的精度提供参考.     

地名识别与匹配的概率统计方法

建立了一个试验用地名库和地理语料库,在此基础上构建对地名用字可信度的统计分析模型。通过分析地名在中文文档中的使用习惯和规律,总结出经常与地名一起使用的且具有地名指示含义的辅助字或词,以此为基础建立地名识别辅助词词库和地名识别的规则库。对地名库和地理语料库的用字进行统计分析,通过设定地名用字可信度概率阈值和辅助词指示作用对文本中潜在地名进行初步的筛选形成候选地名;在粗筛选产生的候选地名基础上结合地名识别规则进一步确认,以提高地名识别的准确率。     

Intel MKL在Bernese GNSS数据处理中的应用

为提高Bernese GNSS software数据处理效率，将英特尔数学核心函数库(math kernel library，MKL)应用于Bernese 精密定轨数据处理，对比分析多个MKL矩阵求逆函数与Bernese 原有程序的计算效率。使用2019-03全球200个测站北斗/GNSS数据进行实验分析，结果表明，采用参数预消除策略时，参数预消除步骤消耗时间明显大于矩阵求逆，使用MKL处理数据效率提升不明显；而未采用参数预消除策略时，使用MKL矩阵求逆函数可显著提高矩阵求逆效率，其中dpotri函数矩阵求逆计算效率最高，消耗时间平均值为133 s，相比Bernese 原有程序计算速度可提高13倍。     

On seasonal approach to flood frequency modelling. Part II: flood frequency analysis of Polish rivers

The annual peak flow series of Polish rivers are mixtures of summer and winter flows. As Part II of a sequence of two papers, practical aspects of applicability of seasonal approach to flood frequency analysis (FFA) of Polish rivers are discussed. Taking A Two‐Component Extreme Value (TCEV1) model as an example it was shown in the first part that regardless of estimation method, the seasonal approach can give profit in terms of upper quantile estimation accuracy that rises with the return period of the quantile and is the greatest for no seasonal variation. In this part, an assessment of annual maxima (AM) versus seasonal maxima (SM) approach to FFA was carried out with respect to seasonal and annual peak flow series of 38 Polish gauging stations. First, the assumption of mutual independence of the seasonal maxima has been tested. The smoothness of SM and AM empirical probability distribution functions was analysed and compared. The TCEV1 model with seasonally estimated parameters was found to be not appropriate for most Polish data as it considerably underrates the skewness of AM distributions and upper quantile values as well. Consequently, the discrepancies between the SM and AM estimates of TCEV1 are observed. Taking SM and TCEV1 distribution, the dominating season in AM series was confronted with predominant season for extreme floods. The key argument for presumptive superiority of SM approach that SM samples are more statistically homogeneous than AM samples has not been confirmed by the data. An analysis of fitness to SM and AM of Polish datasets made for seven distributions pointed to Pearson (3) distribution as the best for AM and Summer Maxima, whereas it was impossible to select a single best model for winter samples. In the multi‐model approach to FFA, the tree functions, i.e., Pe(3), CD3 and LN3, should be involved for both SM and AM. As the case study, Warsaw gauge on the Vistula River was selected. While most of AM elements are here from winter season, the prevailing majority of extreme annual floods are the summer maxima. The upper quantile estimates got by means of classical annual and two‐season methods happen to be fairly close; what's more they are nearly equal to the quantiles calculated just for the season of dominating extreme floods. Copyright © 2011 John Wiley & Sons, Ltd.     

知识经济时代图书馆人力资源的开发与管理

在知识经济条件下，如何提高图书馆人力资源开发与管理的质量，调动广大图书工作者的积极性发挥他们的创造力，将直接影响到图书馆的发展和服务能力。     

利用复测水准资料寻求反映地壳纯形变的定量指标

地壳纯变形分为剪切变形和扩张变形。在前人研究的基础上提出了仅利用复测水准资料求出描述地壳剪切变形和扩张变形指标的方法和步骤，所得的定量指标不受基准的影响，受测量累积误差的影响亦很小，能客观地反映地壳变形的特征。通过理论和实例证明：以一点周围变形分量的最大值代表该点周围垂直面的变形程度比其平均值更能突出变形信息。最后根据实例计算结果分析了剪切变形分量、扩张变形分量与形变速率、构造地震的关系。     

神经网络专家系统外壳

神经网络专家系统外壳软件,是用于帮助用户迅速开发直观图形解释的人工智能业务应用系统。它以直观的屏幕树图为媒介,实现了正、反向推理机、语义网络、神经元网络、框架结构、知识库管理和算术表达式树图等整体宏观统一;实现了专家系统与人工神经元网络、定性分析与定量计算的统一;无监督分类与监督分类的统一。因此,它的应用范围很广。     

The Martian Nonhydrostatic Components of Moment-of-Inertia

The author puts forward the proposal in this paper that all the terrestrial planets (Venus, the Earth, and Mars) as well as the Moon deviate from hydrostatic equilibrium to some degree. The Earth's level of deviation of these four celestial bodies is minimum, and that of Mars is maximum. Moreover, the author estimates Martian nonhydrostatic components of the principal moments-of-inertia using five models for the interior of Mars. Comparison with other terrestrial planets shows that setting the range of mean moment-of-inertia ratio, I/MR², in 0.345 ~ 0.355for Mars is reasonable. This revised version was published online in July 2006 with corrections to the Cover Date.     

银河系厚盘的本地空间密度

本文利用北银极天区的现代恒星计数资料，采用标准的银河系模型，通过恒星统计积分方程对参数值组合模型的亮度函数进行计数分析，证明了银河系厚盘恒星成份存在的必要性，并进一步得出太阳附近厚盘成份的空间密度的最佳期望值为薄盘密度的０．０４１．